Compared to the control star-forming and quiescent galaxies,
AGN host galaxies have a broad sSFR distribution that
extends to both star-forming and quiescent regions. However,
the interpretation of this result is not straightforward,
because the SFR estimates for AGNs may have larger uncertainties
[1]}.
The velocity dispersion distribution for AGNs is between the
two control samples, suggesting that the supermassive
black hole (SMBH) mass (\(M_{\rm BH}\) ) and the bulge mass of
AGN hosts lie between the star-forming and quiescent populations.
The difference between the AGN host galaxies and the star-forming
galaxies becomes smaller as stellar mass increases. The color and \(D_n4000\) 
distributions show similar trends, with the AGN host galaxies
lying between the star-forming and quiescent populations.
These results are in broad agreement with previous
investigations [2]}, [3]}, which
found that AGN host galaxies tend to be in the green valley.
